The Universe Is Expanding — Question 2

Section 44-10 · Physics pages 7474–7475

Question 2 Converting the Hubble rate exposes its characteristic time For this exercise take H0 = 70 km s−1 Mpc−1, 1 Mpc=3.086 × 1019 km and 1 year=3.156 × 107 s. expansion earlier later Schematic; labels, not drawing lengths, specify the data. (a) Convert H0 to inverse seconds and compute the Hubble time. (b) Find the recession rate for proper distance 50 Mpc in the nearby Hubble-flow approximation.
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Question 2 - Solution Converting the Hubble rate exposes its characteristic time expansion earlier later (a) Method and calculation H0 = 70/(3.086 × 1019) = 2.268 × 10−18 s−1 . H−1 0 = 4.409 × 1017 s = 13.969 Gyr . (b) Interpretation and further calculation v = H0D. v = 70(50) = 3500 km/s . Physical check The Hubble time is a scale, not automatically the age. The present expansion rate alone does not specify expansion history.

Question 2

Converting the Hubble rate exposes its characteristic time

For this exercise take H0=70H_0=70 km s−1^{-1} Mpc−1^{-1}, 1 Mpc=3.086×10193.086\times10^{19} km and 1 year=3.156×1073.156\times10^7 s.

Diagram shown in the original SVG worksheet.

  1. Convert H0 to inverse seconds and compute the Hubble time.

  2. Find the recession rate for proper distance 50 Mpc in the nearby Hubble-flow approximation.

Question 2 - Solution

Converting the Hubble rate exposes its characteristic time

Diagram shown in the original SVG worksheet.

(a) Method and calculation

H0=70/(3.086×1019)=2.268×10−18s−1.\boxed{H_0=70/(3.086\times10^{19})=2.268\times10^{-18}\ {\mathrm{s}}^{-1}}.H0−1=4.409×1017s=13.969Gyr.\boxed{H_0^{-1}=4.409\times10^{17}\ {\mathrm{s}}=13.969\ {\mathrm{Gyr}}}.

(b) Interpretation and further calculation

v=H0D.v=H_0D.v=70(50)=3500km/s.\boxed{v=70(50)=3500\ {\mathrm{km/s}}}.

Physical check

The Hubble time is a scale, not automatically the age. The present expansion rate alone does not specify expansion history.